Moreover, we focused on the Hubble and the GO cutoffs and found
out that these cutoffs may also lead to HDE models compatible with
observations. In fact, we saw that, unlike the non-interacting HDE
model with the Hubble cutoff [1]}, it is possible to have
\(\omega _D<0\)  and \(q<0\)  in the interacting case. In addition, our
study shows that the model with the GO cutoff can predict the
universe transition from a deceleration phase to an acceleration
one at around \(z\approx 0\cdot 6\) . We finally found out that the EOS
of the model with GO cutoff may also cross the phantom line.
We also thank Shiraz University Research Council.
This work has been supported financially by Research Institute for
Astronomy & Astrophysics of Maragha (RIAAM), Iran.
